output
20022026
most citedThe Gaia mission

7.1k citations

Showing 2021 · astro-ph.GAShow all

65 papers · 2 filters

astro-ph.GA2021★ 3 cited

Near-IR narrow-band imaging with CIRCE at the Gran Telescopio Canarias: Searching for Ly-emitters at

C. Cabello, J. Gallego, N. Cardiel +8

Identifying very high-redshift galaxies is crucial for understanding the formation and evolution of galaxies. However, many questions still remain, and the uncertainty on the epoch…

astro-ph.GA2021★ 2 cited

HARMONI view of the host galaxies of active galactic nuclei around cosmic noon: Resolved stellar morpho-kinematics and the M- relation

Begoña Garcia-Lorenzo, Ana Monreal-Ibero, Miguel Pereira-Santaella +4

Context. The formation and evolution of galaxies appear linked to the growth of supermassive black holes, as evidenced by empirical scaling relations in nearby galaxies. Understand…

astro-ph.GA2021

Galactic Star Formation with NIKA2 (GASTON): Evidence of mass accretion onto dense clumps

A. J. Rigby, R. Adam, P. Ade +49

High-mass stars () play a crucial role in the evolution of galaxies, and so it is imperative that we understand how they are formed. We have used the New…

astro-ph.GA2021★ 13 cited

Differential attenuation in star-forming galaxies at 0.3 1.5 in the SHARDS/CANDELS field

L. Rodríguez-Muñoz, G. Rodighiero, P. G. Pérez-González +21

We use a sample of 706 galaxies, selected as [OII]3727 ([OII]) emitters in the Survey for High- Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to stud…

astro-ph.GA2021★ 5 cited

Temperature Discrepancy with Photoionization Models of the Narrow Line Region

Luc Binette, Montserrat Villar Martín, Gladis Magris C. +4

Using published work on the Narrow Line Region of Active Nuclei, we make a comparison of the observed [O III] ratio observed among quasars, Seyfert 2's and spatially…

astro-ph.GA2021★ 36 cited

BASS XXIX: The near-infrared view of the BLR: the effects of obscuration in BLR characterisation

Ricci F., Treister E., Bauer F. E. +24

Virial black hole mass () determination directly involves knowing the broad line region (BLR) clouds velocity distribution, their distance from the central supermassive bla…